Suzaku broad-band spectroscopy of RX J1347.5-1145: Constraints on the extremely hot gas and non-thermal emission

Astronomy and Astrophysics

Volumn 491, Issue 2, 2008, Pages 363-377

  Ota, N ^a,b   Murase, K ^c   Kitayama, T ^d   Komatsu, E ^e   Hattori, M ^f   Matsuo, H ^g   Oshima, T ^g   Suto, Y ^h   Yoshikawa, K ⁱ  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c SAITAMA UNIVERSITY   (Japan)

^d TOHO UNIVERSITY   (Japan)

^e UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^f TOHOKU UNIVERSITY   (Japan)

^g NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^h UNIVERSITY OF TOKYO   (Japan)

ⁱ UNIVERSITY OF TSUKUBA   (Japan)

Author keywords

cosmology: observations; Galaxies: clusters: individual: RX J1347.5 1145; galaxies: intergalactic medium; X rays: galaxies: clusters

Indexed keywords

COMPTON SCATTERING; COSMOLOGY; ELECTROMAGNETIC WAVES; EMISSION SPECTROSCOPY; GALAXIES; GASES; LEAKAGE (FLUID); MAGNETIC FIELDS; MERGERS AND ACQUISITIONS; MERGING; RELATIVITY; SPECTRUM ANALYZERS; SPONTANEOUS EMISSION; X RAYS;

BACKGROUND ESTIMATIONS; CHANDRA; CONFIDENCE LEVELS; CONTINUUM EMISSIONS; COSMOLOGY: OBSERVATIONS; GALAXIES: CLUSTERS: INDIVIDUAL: RX J1347.5-1145; GALAXIES: INTERGALACTIC MEDIUM; HOT COMPONENTS; HOT GASSES; INVERSE COMPTON SCATTERINGS; JOINT ANALYSES; LOWER LIMITS; LUMINOUS GALAXIES; RAY ANALYSES; RELATIVISTIC ELECTRONS; SPECTRAL ANALYSES; SZ EFFECTS; TEMPERATURE MODELS; THERMAL EMISSIONS; UPPER LIMITS; X-RAYS: GALAXIES: CLUSTERS;

X RAY ANALYSIS;

EID: 57049119198     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810122     Document Type: Article

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